Properties of Neon, Magnesium, and Silicon Primary Cosmic Rays Results from the Alpha Magnetic Spectrometer
We report the observation of new properties of primary cosmic rays, neon (Ne), magnesium (Mg), and silicon (Si), measured in the rigidity range 2.15 GV to 3.0 TV with 1.8 × 106 Ne , 2.2 × 106 Mg , and 1.6 × 106 Si nuclei collected by the Alpha Magnetic Spectrometer experiment on the International Sp...
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| Veröffentlicht in: | Phys.Rev.Lett 2020-05, Vol.124 (21), p.1-211102, Article 211102 |
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| creator | Aguilar, M. Ali Cavasonza, L. Ambrosi, G. Arruda, L. Attig, N. Barao, F. Barrin, L. Bartoloni, A. Başeğmez-du Pree, S. Battiston, R. Becker, U. Behlmann, M. Beischer, B. Berdugo, J. Bertucci, B. Bindi, V. de Boer, W. Bollweg, K. Borgia, B. Boschini, M. J. Bourquin, M. Bueno, E. F. Burger, J. Burger, W. J. Burmeister, S. Cai, X. D. Capell, M. Casaus, J. Castellini, G. Cervelli, F. Chang, Y. H. Chen, G. M. Chen, H. S. Chen, Y. Cheng, L. Chou, H. Y. Chouridou, S. Choutko, V. Chung, C. H. Clark, C. Coignet, G. Consolandi, C. Contin, A. Corti, C. Cui, Z. Dadzie, K. Dai, Y. M. Delgado, C. Della Torre, S. Demirköz, M. B. Derome, L. Di Falco, S. Di Felice, V. Díaz, C. Dimiccoli, F. von Doetinchem, P. Dong, F. Donnini, F. Duranti, M. Egorov, A. Eline, A. Feng, J. Fiandrini, E. Fisher, P. Formato, V. Freeman, C. Galaktionov, Y. Gámez, C. García-López, R. J. Gargiulo, C. Gast, H. Gebauer, I. Gervasi, M. Giovacchini, F. Gómez-Coral, D. M. Gong, J. Goy, C. Grabski, V. Grandi, D. Graziani, M. Guo, K. H. Haino, S. Han, K. C. Hashmani, R. K. He, Z. H. Heber, B. Hsieh, T. H. Hu, J. Y. Huang, Z. C. Incagli, M. Jang, W. Y. Jia, Yi Jinchi, H. Kanishev, K. Khiali, B. Kim, G. N. Kirn, Th Konyushikhin, M. Kounina, O. Kounine, A. |
| description | We report the observation of new properties of primary cosmic rays, neon (Ne), magnesium (Mg), and silicon (Si), measured in the rigidity range 2.15 GV to 3.0 TV with 1.8 × 106 Ne , 2.2 × 106 Mg , and 1.6 × 106 Si nuclei collected by the Alpha Magnetic Spectrometer experiment on the International Space Station. The Ne and Mg spectra have identical rigidity dependence above 3.65 GV. The three spectra have identical rigidity dependence above 86.5 GV, deviate from a single power law above 200 GV, and harden in an identical way. Unexpectedly, above 86.5 GV the rigidity dependence of primary cosmic rays Ne, Mg, and Si spectra is different from the rigidity dependence of primary cosmic rays He, C, and O. This shows that the Ne, Mg, and Si and He, C, and O are two different classes of primary cosmic rays. |
| doi_str_mv | 10.1103/PhysRevLett.124.211102 |
| format | Article |
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J. ; Bourquin, M. ; Bueno, E. F. ; Burger, J. ; Burger, W. J. ; Burmeister, S. ; Cai, X. D. ; Capell, M. ; Casaus, J. ; Castellini, G. ; Cervelli, F. ; Chang, Y. H. ; Chen, G. M. ; Chen, H. S. ; Chen, Y. ; Cheng, L. ; Chou, H. Y. ; Chouridou, S. ; Choutko, V. ; Chung, C. H. ; Clark, C. ; Coignet, G. ; Consolandi, C. ; Contin, A. ; Corti, C. ; Cui, Z. ; Dadzie, K. ; Dai, Y. M. ; Delgado, C. ; Della Torre, S. ; Demirköz, M. B. ; Derome, L. ; Di Falco, S. ; Di Felice, V. ; Díaz, C. ; Dimiccoli, F. ; von Doetinchem, P. ; Dong, F. ; Donnini, F. ; Duranti, M. ; Egorov, A. ; Eline, A. ; Feng, J. ; Fiandrini, E. ; Fisher, P. ; Formato, V. ; Freeman, C. ; Galaktionov, Y. ; Gámez, C. ; García-López, R. J. ; Gargiulo, C. ; Gast, H. ; Gebauer, I. ; Gervasi, M. ; Giovacchini, F. ; Gómez-Coral, D. M. ; Gong, J. ; Goy, C. ; Grabski, V. ; Grandi, D. ; Graziani, M. ; Guo, K. H. ; Haino, S. ; Han, K. C. ; Hashmani, R. K. ; He, Z. H. ; Heber, B. ; Hsieh, T. H. ; Hu, J. Y. ; Huang, Z. C. ; Incagli, M. ; Jang, W. Y. ; Jia, Yi ; Jinchi, H. ; Kanishev, K. ; Khiali, B. ; Kim, G. N. ; Kirn, Th ; Konyushikhin, M. ; Kounina, O. ; Kounine, A.</creator><creatorcontrib>Aguilar, M. ; Ali Cavasonza, L. ; Ambrosi, G. ; Arruda, L. ; Attig, N. ; Barao, F. ; Barrin, L. ; Bartoloni, A. ; Başeğmez-du Pree, S. ; Battiston, R. ; Becker, U. ; Behlmann, M. ; Beischer, B. ; Berdugo, J. ; Bertucci, B. ; Bindi, V. ; de Boer, W. ; Bollweg, K. ; Borgia, B. ; Boschini, M. J. ; Bourquin, M. ; Bueno, E. F. ; Burger, J. ; Burger, W. J. ; Burmeister, S. ; Cai, X. D. ; Capell, M. ; Casaus, J. ; Castellini, G. ; Cervelli, F. ; Chang, Y. H. ; Chen, G. M. ; Chen, H. S. ; Chen, Y. ; Cheng, L. ; Chou, H. Y. ; Chouridou, S. ; Choutko, V. ; Chung, C. H. ; Clark, C. ; Coignet, G. ; Consolandi, C. ; Contin, A. ; Corti, C. ; Cui, Z. ; Dadzie, K. ; Dai, Y. M. ; Delgado, C. ; Della Torre, S. ; Demirköz, M. 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N. ; Kirn, Th ; Konyushikhin, M. ; Kounina, O. ; Kounine, A. ; AMS Collaboration</creatorcontrib><description>We report the observation of new properties of primary cosmic rays, neon (Ne), magnesium (Mg), and silicon (Si), measured in the rigidity range 2.15 GV to 3.0 TV with 1.8 × 106 Ne , 2.2 × 106 Mg , and 1.6 × 106 Si nuclei collected by the Alpha Magnetic Spectrometer experiment on the International Space Station. The Ne and Mg spectra have identical rigidity dependence above 3.65 GV. The three spectra have identical rigidity dependence above 86.5 GV, deviate from a single power law above 200 GV, and harden in an identical way. Unexpectedly, above 86.5 GV the rigidity dependence of primary cosmic rays Ne, Mg, and Si spectra is different from the rigidity dependence of primary cosmic rays He, C, and O. This shows that the Ne, Mg, and Si and He, C, and O are two different classes of primary cosmic rays.</description><identifier>ISSN: 0031-9007</identifier><identifier>EISSN: 1079-7114</identifier><identifier>DOI: 10.1103/PhysRevLett.124.211102</identifier><language>eng</language><publisher>College Park: American Physical Society</publisher><subject>Alpha rays ; Astrophysics ; Cosmic rays ; Dependence ; Instrumentation and Detectors ; International Space Station ; Magnesium ; Magnetic properties ; Neon ; Physics ; Primary cosmic rays ; Rigidity ; Silicon ; Spectra</subject><ispartof>Phys.Rev.Lett, 2020-05, Vol.124 (21), p.1-211102, Article 211102</ispartof><rights>Copyright American Physical Society May 29, 2020</rights><rights>Distributed under a Creative Commons Attribution 4.0 International License</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c530t-4dd45b1d002f53eaf0b1763c0e4b748ae00ad4058a824e9d0888238b212f6063</citedby><cites>FETCH-LOGICAL-c530t-4dd45b1d002f53eaf0b1763c0e4b748ae00ad4058a824e9d0888238b212f6063</cites><orcidid>0000-0002-9394-2392 ; 0000-0002-5331-0606 ; 0000-0001-6725-5399 ; 0000-0003-0960-5658 ; 0000-0002-1558-4948 ; 0000000178317460</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>230,314,776,780,881,2863,2864,27901,27902</link.rule.ids><backlink>$$Uhttps://hal.science/hal-02870846$$DView record in HAL$$Hfree_for_read</backlink><backlink>$$Uhttps://www.osti.gov/biblio/1631208$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Aguilar, M.</creatorcontrib><creatorcontrib>Ali Cavasonza, L.</creatorcontrib><creatorcontrib>Ambrosi, G.</creatorcontrib><creatorcontrib>Arruda, L.</creatorcontrib><creatorcontrib>Attig, N.</creatorcontrib><creatorcontrib>Barao, F.</creatorcontrib><creatorcontrib>Barrin, L.</creatorcontrib><creatorcontrib>Bartoloni, A.</creatorcontrib><creatorcontrib>Başeğmez-du Pree, S.</creatorcontrib><creatorcontrib>Battiston, R.</creatorcontrib><creatorcontrib>Becker, U.</creatorcontrib><creatorcontrib>Behlmann, M.</creatorcontrib><creatorcontrib>Beischer, B.</creatorcontrib><creatorcontrib>Berdugo, J.</creatorcontrib><creatorcontrib>Bertucci, B.</creatorcontrib><creatorcontrib>Bindi, V.</creatorcontrib><creatorcontrib>de Boer, W.</creatorcontrib><creatorcontrib>Bollweg, K.</creatorcontrib><creatorcontrib>Borgia, B.</creatorcontrib><creatorcontrib>Boschini, M. 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H.</creatorcontrib><creatorcontrib>Clark, C.</creatorcontrib><creatorcontrib>Coignet, G.</creatorcontrib><creatorcontrib>Consolandi, C.</creatorcontrib><creatorcontrib>Contin, A.</creatorcontrib><creatorcontrib>Corti, C.</creatorcontrib><creatorcontrib>Cui, Z.</creatorcontrib><creatorcontrib>Dadzie, K.</creatorcontrib><creatorcontrib>Dai, Y. M.</creatorcontrib><creatorcontrib>Delgado, C.</creatorcontrib><creatorcontrib>Della Torre, S.</creatorcontrib><creatorcontrib>Demirköz, M. B.</creatorcontrib><creatorcontrib>Derome, L.</creatorcontrib><creatorcontrib>Di Falco, S.</creatorcontrib><creatorcontrib>Di Felice, V.</creatorcontrib><creatorcontrib>Díaz, C.</creatorcontrib><creatorcontrib>Dimiccoli, F.</creatorcontrib><creatorcontrib>von Doetinchem, P.</creatorcontrib><creatorcontrib>Dong, F.</creatorcontrib><creatorcontrib>Donnini, F.</creatorcontrib><creatorcontrib>Duranti, M.</creatorcontrib><creatorcontrib>Egorov, A.</creatorcontrib><creatorcontrib>Eline, A.</creatorcontrib><creatorcontrib>Feng, J.</creatorcontrib><creatorcontrib>Fiandrini, E.</creatorcontrib><creatorcontrib>Fisher, P.</creatorcontrib><creatorcontrib>Formato, V.</creatorcontrib><creatorcontrib>Freeman, C.</creatorcontrib><creatorcontrib>Galaktionov, Y.</creatorcontrib><creatorcontrib>Gámez, C.</creatorcontrib><creatorcontrib>García-López, R. J.</creatorcontrib><creatorcontrib>Gargiulo, C.</creatorcontrib><creatorcontrib>Gast, H.</creatorcontrib><creatorcontrib>Gebauer, I.</creatorcontrib><creatorcontrib>Gervasi, M.</creatorcontrib><creatorcontrib>Giovacchini, F.</creatorcontrib><creatorcontrib>Gómez-Coral, D. M.</creatorcontrib><creatorcontrib>Gong, J.</creatorcontrib><creatorcontrib>Goy, C.</creatorcontrib><creatorcontrib>Grabski, V.</creatorcontrib><creatorcontrib>Grandi, D.</creatorcontrib><creatorcontrib>Graziani, M.</creatorcontrib><creatorcontrib>Guo, K. H.</creatorcontrib><creatorcontrib>Haino, S.</creatorcontrib><creatorcontrib>Han, K. C.</creatorcontrib><creatorcontrib>Hashmani, R. K.</creatorcontrib><creatorcontrib>He, Z. H.</creatorcontrib><creatorcontrib>Heber, B.</creatorcontrib><creatorcontrib>Hsieh, T. H.</creatorcontrib><creatorcontrib>Hu, J. Y.</creatorcontrib><creatorcontrib>Huang, Z. C.</creatorcontrib><creatorcontrib>Incagli, M.</creatorcontrib><creatorcontrib>Jang, W. Y.</creatorcontrib><creatorcontrib>Jia, Yi</creatorcontrib><creatorcontrib>Jinchi, H.</creatorcontrib><creatorcontrib>Kanishev, K.</creatorcontrib><creatorcontrib>Khiali, B.</creatorcontrib><creatorcontrib>Kim, G. N.</creatorcontrib><creatorcontrib>Kirn, Th</creatorcontrib><creatorcontrib>Konyushikhin, M.</creatorcontrib><creatorcontrib>Kounina, O.</creatorcontrib><creatorcontrib>Kounine, A.</creatorcontrib><creatorcontrib>AMS Collaboration</creatorcontrib><title>Properties of Neon, Magnesium, and Silicon Primary Cosmic Rays Results from the Alpha Magnetic Spectrometer</title><title>Phys.Rev.Lett</title><description>We report the observation of new properties of primary cosmic rays, neon (Ne), magnesium (Mg), and silicon (Si), measured in the rigidity range 2.15 GV to 3.0 TV with 1.8 × 106 Ne , 2.2 × 106 Mg , and 1.6 × 106 Si nuclei collected by the Alpha Magnetic Spectrometer experiment on the International Space Station. The Ne and Mg spectra have identical rigidity dependence above 3.65 GV. The three spectra have identical rigidity dependence above 86.5 GV, deviate from a single power law above 200 GV, and harden in an identical way. Unexpectedly, above 86.5 GV the rigidity dependence of primary cosmic rays Ne, Mg, and Si spectra is different from the rigidity dependence of primary cosmic rays He, C, and O. This shows that the Ne, Mg, and Si and He, C, and O are two different classes of primary cosmic rays.</description><subject>Alpha rays</subject><subject>Astrophysics</subject><subject>Cosmic rays</subject><subject>Dependence</subject><subject>Instrumentation and Detectors</subject><subject>International Space Station</subject><subject>Magnesium</subject><subject>Magnetic properties</subject><subject>Neon</subject><subject>Physics</subject><subject>Primary cosmic rays</subject><subject>Rigidity</subject><subject>Silicon</subject><subject>Spectra</subject><issn>0031-9007</issn><issn>1079-7114</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2020</creationdate><recordtype>article</recordtype><recordid>eNpd0VGL1DAQB_AiCq6nX0GCvihc15kkbbOPy6J3wqrL3r2HbDu1OdumJunBfnuzVA7xKTD5MfyHf5a9RVgjgvh06M7hSI97inGNXK45pjF_lq0Qqk1eIcrn2QpAYL4BqF5mr0J4AADkpVplvw7eTeSjpcBcy76TG6_ZN_NzpGDn4ZqZsWF3tre1G9nB28H4M9u5MNiaHc05sCOFuY-Btd4NLHbEtv3UmWVDTOhuojqmP4rkX2cvWtMHevP3vcruv3y-393m-x83X3fbfV4XAmIum0YWJ2wAeFsIMi2csCpFDSRPlVSGAEwjoVBGcUmbBpRSXKgTR96WUIqr7N2y1oVodahtpLpL-ceURGMpkINK6OOCOtPraTlMO2P17XavLzPgqgIly0dM9sNiJ-9-zxSiHmyoqe_NSG4OmkvkGyWVkIm-_48-uNmP6dqLwmojRXFR5aJq70Lw1D4lQNCXTvU_nerUqV46FX8AzL6Vpg</recordid><startdate>20200529</startdate><enddate>20200529</enddate><creator>Aguilar, M.</creator><creator>Ali Cavasonza, L.</creator><creator>Ambrosi, G.</creator><creator>Arruda, L.</creator><creator>Attig, N.</creator><creator>Barao, F.</creator><creator>Barrin, L.</creator><creator>Bartoloni, A.</creator><creator>Başeğmez-du Pree, S.</creator><creator>Battiston, R.</creator><creator>Becker, U.</creator><creator>Behlmann, M.</creator><creator>Beischer, B.</creator><creator>Berdugo, J.</creator><creator>Bertucci, B.</creator><creator>Bindi, V.</creator><creator>de Boer, W.</creator><creator>Bollweg, K.</creator><creator>Borgia, B.</creator><creator>Boschini, M. 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N.</creator><creator>Kirn, Th</creator><creator>Konyushikhin, M.</creator><creator>Kounina, O.</creator><creator>Kounine, A.</creator><general>American Physical Society</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7U5</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope><scope>7X8</scope><scope>1XC</scope><scope>OTOTI</scope><orcidid>https://orcid.org/0000-0002-9394-2392</orcidid><orcidid>https://orcid.org/0000-0002-5331-0606</orcidid><orcidid>https://orcid.org/0000-0001-6725-5399</orcidid><orcidid>https://orcid.org/0000-0003-0960-5658</orcidid><orcidid>https://orcid.org/0000-0002-1558-4948</orcidid><orcidid>https://orcid.org/0000000178317460</orcidid></search><sort><creationdate>20200529</creationdate><title>Properties of Neon, Magnesium, and Silicon Primary Cosmic Rays Results from the Alpha Magnetic Spectrometer</title><author>Aguilar, M. ; Ali Cavasonza, L. ; Ambrosi, G. ; Arruda, L. ; Attig, N. ; Barao, F. ; Barrin, L. ; Bartoloni, A. ; Başeğmez-du Pree, S. ; Battiston, R. ; Becker, U. ; Behlmann, M. ; Beischer, B. ; Berdugo, J. ; Bertucci, B. ; Bindi, V. ; de Boer, W. ; Bollweg, K. ; Borgia, B. ; Boschini, M. J. ; Bourquin, M. ; Bueno, E. F. ; Burger, J. ; Burger, W. J. ; Burmeister, S. ; Cai, X. D. ; Capell, M. ; Casaus, J. ; Castellini, G. ; Cervelli, F. ; Chang, Y. H. ; Chen, G. M. ; Chen, H. S. ; Chen, Y. ; Cheng, L. ; Chou, H. Y. ; Chouridou, S. ; Choutko, V. ; Chung, C. H. ; Clark, C. ; Coignet, G. ; Consolandi, C. ; Contin, A. ; Corti, C. ; Cui, Z. ; Dadzie, K. ; Dai, Y. M. ; Delgado, C. ; Della Torre, S. ; Demirköz, M. B. ; Derome, L. ; Di Falco, S. ; Di Felice, V. ; Díaz, C. ; Dimiccoli, F. ; von Doetinchem, P. ; Dong, F. ; Donnini, F. ; Duranti, M. ; Egorov, A. ; Eline, A. ; Feng, J. ; Fiandrini, E. ; Fisher, P. ; Formato, V. ; Freeman, C. ; Galaktionov, Y. ; Gámez, C. ; García-López, R. J. ; Gargiulo, C. ; Gast, H. ; Gebauer, I. ; Gervasi, M. ; Giovacchini, F. ; Gómez-Coral, D. M. ; Gong, J. ; Goy, C. ; Grabski, V. ; Grandi, D. ; Graziani, M. ; Guo, K. H. ; Haino, S. ; Han, K. C. ; Hashmani, R. K. ; He, Z. H. ; Heber, B. ; Hsieh, T. H. ; Hu, J. Y. ; Huang, Z. C. ; Incagli, M. ; Jang, W. Y. ; Jia, Yi ; Jinchi, H. ; Kanishev, K. ; Khiali, B. ; Kim, G. N. ; Kirn, Th ; Konyushikhin, M. ; Kounina, O. ; Kounine, A.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c530t-4dd45b1d002f53eaf0b1763c0e4b748ae00ad4058a824e9d0888238b212f6063</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2020</creationdate><topic>Alpha rays</topic><topic>Astrophysics</topic><topic>Cosmic rays</topic><topic>Dependence</topic><topic>Instrumentation and Detectors</topic><topic>International Space Station</topic><topic>Magnesium</topic><topic>Magnetic properties</topic><topic>Neon</topic><topic>Physics</topic><topic>Primary cosmic rays</topic><topic>Rigidity</topic><topic>Silicon</topic><topic>Spectra</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Aguilar, M.</creatorcontrib><creatorcontrib>Ali Cavasonza, L.</creatorcontrib><creatorcontrib>Ambrosi, G.</creatorcontrib><creatorcontrib>Arruda, L.</creatorcontrib><creatorcontrib>Attig, N.</creatorcontrib><creatorcontrib>Barao, F.</creatorcontrib><creatorcontrib>Barrin, L.</creatorcontrib><creatorcontrib>Bartoloni, A.</creatorcontrib><creatorcontrib>Başeğmez-du Pree, S.</creatorcontrib><creatorcontrib>Battiston, R.</creatorcontrib><creatorcontrib>Becker, U.</creatorcontrib><creatorcontrib>Behlmann, M.</creatorcontrib><creatorcontrib>Beischer, B.</creatorcontrib><creatorcontrib>Berdugo, J.</creatorcontrib><creatorcontrib>Bertucci, B.</creatorcontrib><creatorcontrib>Bindi, V.</creatorcontrib><creatorcontrib>de Boer, W.</creatorcontrib><creatorcontrib>Bollweg, K.</creatorcontrib><creatorcontrib>Borgia, B.</creatorcontrib><creatorcontrib>Boschini, M. J.</creatorcontrib><creatorcontrib>Bourquin, M.</creatorcontrib><creatorcontrib>Bueno, E. F.</creatorcontrib><creatorcontrib>Burger, J.</creatorcontrib><creatorcontrib>Burger, W. J.</creatorcontrib><creatorcontrib>Burmeister, S.</creatorcontrib><creatorcontrib>Cai, X. D.</creatorcontrib><creatorcontrib>Capell, M.</creatorcontrib><creatorcontrib>Casaus, J.</creatorcontrib><creatorcontrib>Castellini, G.</creatorcontrib><creatorcontrib>Cervelli, F.</creatorcontrib><creatorcontrib>Chang, Y. H.</creatorcontrib><creatorcontrib>Chen, G. M.</creatorcontrib><creatorcontrib>Chen, H. S.</creatorcontrib><creatorcontrib>Chen, Y.</creatorcontrib><creatorcontrib>Cheng, L.</creatorcontrib><creatorcontrib>Chou, H. Y.</creatorcontrib><creatorcontrib>Chouridou, S.</creatorcontrib><creatorcontrib>Choutko, V.</creatorcontrib><creatorcontrib>Chung, C. H.</creatorcontrib><creatorcontrib>Clark, C.</creatorcontrib><creatorcontrib>Coignet, G.</creatorcontrib><creatorcontrib>Consolandi, C.</creatorcontrib><creatorcontrib>Contin, A.</creatorcontrib><creatorcontrib>Corti, C.</creatorcontrib><creatorcontrib>Cui, Z.</creatorcontrib><creatorcontrib>Dadzie, K.</creatorcontrib><creatorcontrib>Dai, Y. M.</creatorcontrib><creatorcontrib>Delgado, C.</creatorcontrib><creatorcontrib>Della Torre, S.</creatorcontrib><creatorcontrib>Demirköz, M. B.</creatorcontrib><creatorcontrib>Derome, L.</creatorcontrib><creatorcontrib>Di Falco, S.</creatorcontrib><creatorcontrib>Di Felice, V.</creatorcontrib><creatorcontrib>Díaz, C.</creatorcontrib><creatorcontrib>Dimiccoli, F.</creatorcontrib><creatorcontrib>von Doetinchem, P.</creatorcontrib><creatorcontrib>Dong, F.</creatorcontrib><creatorcontrib>Donnini, F.</creatorcontrib><creatorcontrib>Duranti, M.</creatorcontrib><creatorcontrib>Egorov, A.</creatorcontrib><creatorcontrib>Eline, A.</creatorcontrib><creatorcontrib>Feng, J.</creatorcontrib><creatorcontrib>Fiandrini, E.</creatorcontrib><creatorcontrib>Fisher, P.</creatorcontrib><creatorcontrib>Formato, V.</creatorcontrib><creatorcontrib>Freeman, C.</creatorcontrib><creatorcontrib>Galaktionov, Y.</creatorcontrib><creatorcontrib>Gámez, C.</creatorcontrib><creatorcontrib>García-López, R. J.</creatorcontrib><creatorcontrib>Gargiulo, C.</creatorcontrib><creatorcontrib>Gast, H.</creatorcontrib><creatorcontrib>Gebauer, I.</creatorcontrib><creatorcontrib>Gervasi, M.</creatorcontrib><creatorcontrib>Giovacchini, F.</creatorcontrib><creatorcontrib>Gómez-Coral, D. M.</creatorcontrib><creatorcontrib>Gong, J.</creatorcontrib><creatorcontrib>Goy, C.</creatorcontrib><creatorcontrib>Grabski, V.</creatorcontrib><creatorcontrib>Grandi, D.</creatorcontrib><creatorcontrib>Graziani, M.</creatorcontrib><creatorcontrib>Guo, K. H.</creatorcontrib><creatorcontrib>Haino, S.</creatorcontrib><creatorcontrib>Han, K. C.</creatorcontrib><creatorcontrib>Hashmani, R. K.</creatorcontrib><creatorcontrib>He, Z. H.</creatorcontrib><creatorcontrib>Heber, B.</creatorcontrib><creatorcontrib>Hsieh, T. H.</creatorcontrib><creatorcontrib>Hu, J. Y.</creatorcontrib><creatorcontrib>Huang, Z. C.</creatorcontrib><creatorcontrib>Incagli, M.</creatorcontrib><creatorcontrib>Jang, W. Y.</creatorcontrib><creatorcontrib>Jia, Yi</creatorcontrib><creatorcontrib>Jinchi, H.</creatorcontrib><creatorcontrib>Kanishev, K.</creatorcontrib><creatorcontrib>Khiali, B.</creatorcontrib><creatorcontrib>Kim, G. N.</creatorcontrib><creatorcontrib>Kirn, Th</creatorcontrib><creatorcontrib>Konyushikhin, M.</creatorcontrib><creatorcontrib>Kounina, O.</creatorcontrib><creatorcontrib>Kounine, A.</creatorcontrib><creatorcontrib>AMS Collaboration</creatorcontrib><collection>CrossRef</collection><collection>Solid State and Superconductivity Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>MEDLINE - Academic</collection><collection>Hyper Article en Ligne (HAL)</collection><collection>OSTI.GOV</collection><jtitle>Phys.Rev.Lett</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Aguilar, M.</au><au>Ali Cavasonza, L.</au><au>Ambrosi, G.</au><au>Arruda, L.</au><au>Attig, N.</au><au>Barao, F.</au><au>Barrin, L.</au><au>Bartoloni, A.</au><au>Başeğmez-du Pree, S.</au><au>Battiston, R.</au><au>Becker, U.</au><au>Behlmann, M.</au><au>Beischer, B.</au><au>Berdugo, J.</au><au>Bertucci, B.</au><au>Bindi, V.</au><au>de Boer, W.</au><au>Bollweg, K.</au><au>Borgia, B.</au><au>Boschini, M. J.</au><au>Bourquin, M.</au><au>Bueno, E. F.</au><au>Burger, J.</au><au>Burger, W. J.</au><au>Burmeister, S.</au><au>Cai, X. D.</au><au>Capell, M.</au><au>Casaus, J.</au><au>Castellini, G.</au><au>Cervelli, F.</au><au>Chang, Y. H.</au><au>Chen, G. M.</au><au>Chen, H. S.</au><au>Chen, Y.</au><au>Cheng, L.</au><au>Chou, H. Y.</au><au>Chouridou, S.</au><au>Choutko, V.</au><au>Chung, C. H.</au><au>Clark, C.</au><au>Coignet, G.</au><au>Consolandi, C.</au><au>Contin, A.</au><au>Corti, C.</au><au>Cui, Z.</au><au>Dadzie, K.</au><au>Dai, Y. M.</au><au>Delgado, C.</au><au>Della Torre, S.</au><au>Demirköz, M. B.</au><au>Derome, L.</au><au>Di Falco, S.</au><au>Di Felice, V.</au><au>Díaz, C.</au><au>Dimiccoli, F.</au><au>von Doetinchem, P.</au><au>Dong, F.</au><au>Donnini, F.</au><au>Duranti, M.</au><au>Egorov, A.</au><au>Eline, A.</au><au>Feng, J.</au><au>Fiandrini, E.</au><au>Fisher, P.</au><au>Formato, V.</au><au>Freeman, C.</au><au>Galaktionov, Y.</au><au>Gámez, C.</au><au>García-López, R. J.</au><au>Gargiulo, C.</au><au>Gast, H.</au><au>Gebauer, I.</au><au>Gervasi, M.</au><au>Giovacchini, F.</au><au>Gómez-Coral, D. M.</au><au>Gong, J.</au><au>Goy, C.</au><au>Grabski, V.</au><au>Grandi, D.</au><au>Graziani, M.</au><au>Guo, K. H.</au><au>Haino, S.</au><au>Han, K. C.</au><au>Hashmani, R. K.</au><au>He, Z. H.</au><au>Heber, B.</au><au>Hsieh, T. H.</au><au>Hu, J. Y.</au><au>Huang, Z. C.</au><au>Incagli, M.</au><au>Jang, W. Y.</au><au>Jia, Yi</au><au>Jinchi, H.</au><au>Kanishev, K.</au><au>Khiali, B.</au><au>Kim, G. N.</au><au>Kirn, Th</au><au>Konyushikhin, M.</au><au>Kounina, O.</au><au>Kounine, A.</au><aucorp>AMS Collaboration</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Properties of Neon, Magnesium, and Silicon Primary Cosmic Rays Results from the Alpha Magnetic Spectrometer</atitle><jtitle>Phys.Rev.Lett</jtitle><date>2020-05-29</date><risdate>2020</risdate><volume>124</volume><issue>21</issue><spage>1</spage><epage>211102</epage><pages>1-211102</pages><artnum>211102</artnum><issn>0031-9007</issn><eissn>1079-7114</eissn><abstract>We report the observation of new properties of primary cosmic rays, neon (Ne), magnesium (Mg), and silicon (Si), measured in the rigidity range 2.15 GV to 3.0 TV with 1.8 × 106 Ne , 2.2 × 106 Mg , and 1.6 × 106 Si nuclei collected by the Alpha Magnetic Spectrometer experiment on the International Space Station. The Ne and Mg spectra have identical rigidity dependence above 3.65 GV. The three spectra have identical rigidity dependence above 86.5 GV, deviate from a single power law above 200 GV, and harden in an identical way. Unexpectedly, above 86.5 GV the rigidity dependence of primary cosmic rays Ne, Mg, and Si spectra is different from the rigidity dependence of primary cosmic rays He, C, and O. This shows that the Ne, Mg, and Si and He, C, and O are two different classes of primary cosmic rays.</abstract><cop>College Park</cop><pub>American Physical Society</pub><doi>10.1103/PhysRevLett.124.211102</doi><orcidid>https://orcid.org/0000-0002-9394-2392</orcidid><orcidid>https://orcid.org/0000-0002-5331-0606</orcidid><orcidid>https://orcid.org/0000-0001-6725-5399</orcidid><orcidid>https://orcid.org/0000-0003-0960-5658</orcidid><orcidid>https://orcid.org/0000-0002-1558-4948</orcidid><orcidid>https://orcid.org/0000000178317460</orcidid><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 0031-9007 |
| ispartof | Phys.Rev.Lett, 2020-05, Vol.124 (21), p.1-211102, Article 211102 |
| issn | 0031-9007 1079-7114 |
| language | eng |
| recordid | cdi_osti_scitechconnect_1631208 |
| source | EZB Electronic Journals Library; APS: American Physical Society E-Journals (Physics) |
| subjects | Alpha rays Astrophysics Cosmic rays Dependence Instrumentation and Detectors International Space Station Magnesium Magnetic properties Neon Physics Primary cosmic rays Rigidity Silicon Spectra |
| title | Properties of Neon, Magnesium, and Silicon Primary Cosmic Rays Results from the Alpha Magnetic Spectrometer |
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